Early Optical Follow-Up Observations of Einstein Probe X-Ray Transients During the First Year

We present early follow-up observations of Einstein Probe (EP) X-ray transients, following its first year of operation. EP is a dedicated wide-field X-ray observatory that is transforming our understanding of the dynamic X-ray universe. During its first year, EP successfully detected a diverse range of high-energy transients—including gamma-ray bursts (GRBs), tidal disruption events (TDEs), and fast X-ray transients (FXTs), besides many stellar flares, disseminating 128 alerts in the aggregate. Ground-based optical follow-up observations, particularly those performed by our BOOTES telescope network, have played a crucial role in multi-wavelength campaigns carried out so far. Out of the 128 events, the BOOTES Network has been able to follow up 58 events, detecting 6 optical counterparts at early times. These complementary optical measurements have enabled rapid identification of counterparts, precise redshift determinations (such as EP250215a at z=4.61), and detailed characterization of the transient phenomena. The synergy between EP’s cutting-edge X-ray monitoring and the essential optical follow-up provided by facilities, such as the above-mentioned BOOTES Global Network or other Spanish ground-based facilities we have access to, underscores the importance and necessity of coordinated observations in the era of time-domain and multi-messenger astrophysics.

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Publication Details

Journal
Galaxies
Published
2025-05-19
DOI
https://doi.org/10.3390/galaxies13030062
Citations
1
Primary Topic
Gamma-ray bursts and supernovae
Type
article
Field-Weighted Citation Impact
1.15

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article

Early Optical Follow-Up Observations of Einstein Probe X-Ray Transients During the First Year

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1 citations
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Gamma-ray bursts and supernovae
1.15
article

Early Optical Follow-Up Observations of Einstein Probe X-Ray Transients During the First Year

Sergiy Guziy, Maria Gritsevich, Carlos J. Pérez-del-Pulgar, Emilio J. Fernández-García, S. S. Wu, Y. D. Hu, Dingrong Xiong, A. J. Castro‐Tirado, R. Sánchez-Ramírez, Ignacio Pérez-García, M. D. Caballero‐García, Bin‐Bin Zhang, Guillermo García Segura
article en
1 citations

Abstract

We present early follow-up observations of Einstein Probe (EP) X-ray transients, following its first year of operation. EP is a dedicated wide-field X-ray observatory that is transforming our understanding of the dynamic X-ray universe. During its first year, EP successfully detected a diverse range of high-energy transients—including gamma-ray bursts (GRBs), tidal disruption events (TDEs), and fast X-ray transients (FXTs), besides many stellar flares, disseminating 128 alerts in the aggregate. Ground-based optical follow-up observations, particularly those performed by our BOOTES telescope network, have played a crucial role in multi-wavelength campaigns carried out so far. Out of the 128 events, the BOOTES Network has been able to follow up 58 events, detecting 6 optical counterparts at early times. These complementary optical measurements have enabled rapid identification of counterparts, precise redshift determinations (such as EP250215a at z=4.61), and detailed characterization of the transient phenomena. The synergy between EP’s cutting-edge X-ray monitoring and the essential optical follow-up provided by facilities, such as the above-mentioned BOOTES Global Network or other Spanish ground-based facilities we have access to, underscores the importance and necessity of coordinated observations in the era of time-domain and multi-messenger astrophysics.

GalaxiesVol. 13(3)
Petro Mohyla Black Sea National University (UA), Ural Federal University (RU), Swedish Institute of Space Physics (SE), University of Helsinki (FI), Consejo Superior de Investigaciones Científicas (ES), Guangxi University (CN), Universidad de Granada (ES), Chinese Academy of Sciences (CN), Yunnan Observatories (CN), Ensenada Institute of Technology (MX), Institute of Physics and Technology (RU), Instituto de Astrofísica de Andalucía (ES), Universidad de Málaga (ES), Nanjing University (CN), Universidad Nacional Autónoma de México (MX)
Ministerio de Ciencia, Innovación y Universidades, Academy of Finland, China Scholarship Council, Ministerio de Ciencia e Innovación, Ural Federal University, Instituto de Astrofísica de Andalucía, Agencia Estatal de Investigación
Openalex Percentile: Top 19%
Gamma-ray bursts and supernovae
1.15
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